High-resolution ammonia mapping of the very young protostellar core Chamaeleon-MMS1

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Volume 564 (April 2014)

A&A, 564 (2014) A99

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Table 6

Results of SED modelling.

Parameter^a	Value^b

χ ² / N _data	85.34 [86.29–95.98]
Inclination, i [°]	69.51 [63.26–87.13]
Stellar age, τ_⋆ [10⁴ yr]	2.65 [2.65–6.95]
Stellar mass, M_⋆ [M_⊙]	0.12 [0.12–0.18]
Stellar temperature, T_⋆ [10³ K]	2.78 [2.78–3.02]
Envelope accretion rate, Ṁ_env [10^-5M_⊙ yr^-1]	4.26 [2.84–4.91]
Disk mass, M_disk [M_⊙]	0.0013 [1.7 × 10^-4–0.0095]
Total luminosity, L_tot [L_⊙]	0.59 [0.43–0.68]
Envelope mass, M_env [M_⊙]	0.88 [0.46–0.88]
Stage	0

Notes.

^(a)

The parameters are described in detail in Robitaille et al. (2006).

^(b)

For each model parameter, the best-fit value is given, followed by a range defined by the minimum and maximum values obtained from the subsequent nine best-fit models.

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